HIRIS — Eos instrument with high spectral and spatial resolution

Jeff Dozier , Alexander F.H. Goetz
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引用次数: 6

Abstract

The High-Resolution Imaging Spectrometer (HIRIS) is a JPL-facility instrument designed for NASA's Earth Observing System (Eos). It will have 10-nm wide spectral bands from 0.4 to 2.5 μm at 30-m spatial resolution over a 24-km swath. The spectral resolution allows identification of many minerals in rocks and soils, important algal pigments in oceans and inland waters, spectral changes associated with plant canopy biochemistry, composition of atmospheric aerosols, and grain size of snow and its contamination by absorbing impurities. The bands will have 12-bit quantization over a dynamic range suitable for bright targets, such as snow. For targets of low brightness, such as water bodies, image-motion compensation will allow gains up to a factor of 8 to increase signal-to-noise ratios. The sensor will be able to point ±26° crosstrack and +52°/−30° downtrack. In the 705-km orbit altitude proposed for Eos, the crosstrack pointing capability will allow 3–4 views during a 16-day revisit cycle.

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具有高光谱和空间分辨率的HIRIS - Eos仪器
高分辨率成像光谱仪(HIRIS)是jpl为NASA地球观测系统(Eos)设计的设备。它将在24公里范围内以30米的空间分辨率具有0.4至2.5 μm的10纳米宽光谱带。光谱分辨率允许识别岩石和土壤中的许多矿物质,海洋和内陆水域中的重要藻类色素,与植物冠层生物化学相关的光谱变化,大气气溶胶的组成,雪的粒度及其吸收杂质的污染。这些波段将在一个适合明亮目标(如雪)的动态范围内进行12位量化。对于低亮度的目标,如水体,图像运动补偿将使增益达到8倍,以增加信噪比。传感器将能够指向±26°的横向轨迹和+52°/ - 30°的向下轨迹。在Eos的705千米轨道高度上,交叉轨道指向能力将允许在16天的重访周期内进行3-4次观测。
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